22.07.2013 Views

Max Planck Institute for Astronomy - Annual Report 2007

Max Planck Institute for Astronomy - Annual Report 2007

Max Planck Institute for Astronomy - Annual Report 2007

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

88 III. Selected Research Areas<br />

III.4 Starburst Clusters in the Milky Way<br />

The majority of stars are born not in isolation, but in<br />

stellar clusters and associations. Interacting galaxies<br />

like the Antennae galaxies are the birthplaces of massive<br />

stellar clusters with several 100,000 to millions of<br />

stars. Over time, these super star clusters are expected<br />

to evolve into globular clusters quite similar to the<br />

150 or so that constitute the Milky Way globular cluster<br />

system, which <strong>for</strong>med about 13 billion years ago.<br />

Among the most extreme star <strong>for</strong>mation environments<br />

in the present-day Milky Way are starburst clusters<br />

with several 10,000 to 100,000 stars. As the stellar population<br />

in starburst clusters contains stars with masses<br />

from 0.1 to 120 solar masses, starburst clusters are<br />

ideal testbeds to study star <strong>for</strong>mation and early stellar<br />

evolution across the entire range of stellar masses.<br />

Fig. III.4.1. Location of the presently known starburst clusters<br />

plotted on a map (courtesy of Wikipedia) of the Milky Way<br />

spiral arm structure. The Sun's orbit is indicated by a black<br />

circle, and the present-day position of the Sun by a yellow<br />

dot. The small inserts show near-infrared observations of the<br />

individual starburst clusters.<br />

Local Spur<br />

Perseus<br />

WD2<br />

Sagittarius<br />

WD1<br />

NGC3603<br />

Starburst clusters with ages of a few million years represent<br />

unique astrophysical laboratories, because they contain,<br />

in a rather homogeneous environment, stars across<br />

the entire stellar mass range from the upper mass cut-off in<br />

the mass function down to the hydrogen burning limit (and<br />

possibly beyond) and with the same metallicity and age.<br />

As such, starburst clusters are the ideal places to study<br />

star <strong>for</strong>mation and to test theories on <strong>for</strong>mation and evolution<br />

of stars and clusters. Unlike interacting galaxies<br />

such as the Antennae galaxies, where hundreds of super<br />

star clusters have been identified, the Milky Way houses<br />

only a handful of starburst clusters. Starburst clusters in<br />

the Antennae, however, are barely resolved, restricting<br />

study to the integrated properties of hundred thousands<br />

of stars. In the Milky Way, on the other hand, starburst<br />

clusters can be resolved into thousands to tens of thousands<br />

of stars, and the properties of each star can be derived<br />

individually.<br />

Galactic Starburst Clusters<br />

Milky Way starburst clusters can be found either in the<br />

galactic center region or in spiral arms. Because of strong<br />

RSGC1<br />

Arches<br />

Galactic<br />

Center<br />

Quintuplet<br />

Norma<br />

Scutum-Crux<br />

Sun’s Orbit<br />

Obscured

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!